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Komiya, Yutaka, Suda, Takuma, Yamada, Shimako, Fujimoto, Masayuki Y. (2020) Are Faint Supernovae Responsible for Carbon-enhanced Metal-poor Stars?. The Astrophysical Journal, 890 (1). 66pp. doi:10.3847/1538-4357/ab67be

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Reference TypeJournal (article/letter/editorial)
TitleAre Faint Supernovae Responsible for Carbon-enhanced Metal-poor Stars?
JournalThe Astrophysical Journal
AuthorsKomiya, YutakaAuthor
Suda, TakumaAuthor
Yamada, ShimakoAuthor
Fujimoto, Masayuki Y.Author
Year2020 (February 12)Volume890
Issue1
PublisherAmerican Astronomical Society
DOIdoi:10.3847/1538-4357/ab67beSearch in ResearchGate
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Mindat Ref. ID3553122Long-form Identifiermindat:1:5:3553122:3
GUID0
Full ReferenceKomiya, Yutaka, Suda, Takuma, Yamada, Shimako, Fujimoto, Masayuki Y. (2020) Are Faint Supernovae Responsible for Carbon-enhanced Metal-poor Stars?. The Astrophysical Journal, 890 (1). 66pp. doi:10.3847/1538-4357/ab67be
Plain TextKomiya, Yutaka, Suda, Takuma, Yamada, Shimako, Fujimoto, Masayuki Y. (2020) Are Faint Supernovae Responsible for Carbon-enhanced Metal-poor Stars?. The Astrophysical Journal, 890 (1). 66pp. doi:10.3847/1538-4357/ab67be
In(2020, February) The Astrophysical Journal Vol. 890 (1) American Astronomical Society

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Yamada, Shimako, Suda, Takuma, Komiya, Yutaka, Aikawa, Masayuki, Fujimoto, Masayuki Y (2023) A comparative study of three modes of s-process nucleosynthesis in extremely metal-poor AGB stars. Publications of the Astronomical Society of Japan, 75 (6) 1145-1167 doi:10.1093/pasj/psad062
Suda, Takuma, Katsuta, Yutaka, Yamada, Shimako, Suwa, Tamon, Ishizuka, Chikako, Komiya, Yutaka, Sorai, Kazuo, Aikawa, Masayuki, Fujimoto, Masayuki Y. (2008) Stellar Abundances for the Galactic Archeology (SAGA) Database — Compilation of the Characteristics of Known Extremely Metal-Poor Stars. Publications of the Astronomical Society of Japan, 60 (5). 1159-1171 doi:10.1093/pasj/60.5.1159
Komiya, Yutaka, Suda, Takuma, Fujimoto, Masayuki Y. (2016) POPULATION III STARS AROUND THE MILKY WAY. The Astrophysical Journal, 820 (1). 59pp. doi:10.3847/0004-637x/820/1/59
Komiya, Yutaka, Habe, Asao, Suda, Takuma, Fujimoto, Masayuki Y. (2009) HIERARCHICAL FORMATION OF THE GALACTIC HALO AND THE ORIGIN OF HYPER METAL-POOR STARS. The Astrophysical Journal, 696 (1). doi:10.1088/0004-637x/696/1/l79
Komiya, Yutaka, Suda, Takuma, Fujimoto, Masayuki Y. (2009) EARLY-AGE EVOLUTION OF THE MILKY WAY RELATED BY EXTREMELY METAL-POOR STARS. The Astrophysical Journal, 694 (2). 1577-1594 doi:10.1088/0004-637x/694/2/1577
Komiya, Yutaka, Suda, Takuma, Minaguchi, Hiroki, Shigeyama, Toshikazu, Aoki, Wako, Fujimoto, Masayuki Y. (2007) The Origin of Carbon Enhancement and the Initial Mass Function of Extremely Metal‐poor Stars in the Galactic Halo. The Astrophysical Journal, 658 (1). 367-390 doi:10.1086/510826
Komiya, Yutaka, Habe, Asao, Suda, Takuma, Fujimoto, Masayuki Y. (2010) FORMATION HISTORY OF METAL-POOR HALO STARS WITH THE HIERARCHICAL MODEL AND THE EFFECT OF INTERSTELLAR MATTER ACCRETION ON THE MOST METAL-POOR STARS. The Astrophysical Journal, 717 (1). 542-561 doi:10.1088/0004-637x/717/1/542
Suda, Takuma, Yamada, Shimako, Katsuta, Yutaka, Ishizuka, Chikako, Komiya, Yutaka, Nishimura, Takanori, Aoki, Wako, Fujimoto, Masayuki Y. (2009) An overall picture of EMP stars using the stellar abundances for galactic archaeology (SAGA) database. Proceedings of the International Astronomical Union, 5. 90-93 doi:10.1017/s174392131000027x
Komiya, Yutaka, Suda, Takuma, Habe, Asao, Fujimoto, Masayuki (2008) Galactic archeology with extremely metal-poor stars. Proceedings of the International Astronomical Union, 4. 330-335 doi:10.1017/s1743921308025027
Komiya, Yutaka, Yamada, Shimako, Suda, Takuma, Fujimoto, Masayuki Y. (2014) THE NEW MODEL OF CHEMICAL EVOLUTION OFr-PROCESS ELEMENTS BASED ON THE HIERARCHICAL GALAXY FORMATION. I. Ba AND Eu. The Astrophysical Journal, 783 (2). 132pp. doi:10.1088/0004-637x/783/2/132
Komiya, Yutaka, Suda, Takuma, Fujimoto, Masayuki Y. (2015) THE MOST IRON-DEFICIENT STARS AS THE POLLUTED POPULATION III STARS. The Astrophysical Journal, 808 (2). doi:10.1088/2041-8205/808/2/l47
 
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